Our linear models are able to reproduce the observed decrease of spatial growth rate with shear, if we take into account the narrowing of the jet by assuming the meridional wavelength of the perturbations is set by the jet. The decrease in growth rate results from the decrease in meridional wavelengths when the jet is stronger and narrower. Our results hold when surface damping is added. A common suggestion has been that perturbations are weaker when the jet is strong because they move faster out of the unstable storm track region. We find that we need to take into account that the jet narrows when it strengthens, otherwise, the increase of growth rate is strong enough to counteract the effect of increased advection speed.
We also find that when the model basic state is Eady-like (small or zero meridional PV gradients in the troposphere) the short wave cutoff for instability moves to larger waves as shear is increased, due to the accompanying increase in meridional wavenumber. This results in a transition from a regime where upper level perturbations spin up a surface circulation very rapidly and normal mode growth ensues, to a regime where the initial perturbations take a very long time to excite growth. Since waves slow down when a surface perturbation develops, this can explain the observations that the storm track perturbations are more ``upper level'' during strong jet years and their group velocities increase faster than linearly with shear.
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